
Planck 2018 measurements of the low-\(\ell \)  CMB TT, EE, and high-\(\ell \)  TT, TE, EE power spectra, together with the gravitational lensing potential reconstruction [1]}.

The BAO measurements from 6dFGS at \(z=0.106\)  [2]}, SDSS DR7 at \(z=0.15\)  [3]}, BOSS DR12 at \(z=0.38, 0.51\)  and \(0.61\)  [4]}, and the joint constraints from eBOSS DR14 Ly-\(\alpha \)  auto-correlation at \(z=2.34\)  [5]} and cross-correlation at \(z=2.35\)  [6]}.

The measurements of the growth function \(f\sigma _8(z)\)  (FS) from the CMASS and LOWZ galaxy samples of BOSS DR12 at \(z = 0.38\) , \(0.51\) , and \(0.61\)  [4]}.

The Pantheon SNIa catalogue, spanning redshifts \(0.01 < z < 2.3\)  [8]}.

The SH0ES result, modeled with a Gaussian likelihood centered on \(H_0 = 73.2 \pm 1.3\)  km/s/Mpc [9]}; however, choosing a different value that combines various direct measurements would not affect the result, given their small differences.

The KIDS1000+BOSS+2dfLenS weak lensing data, compressed as a split-normal likelihood on the parameter \(S_8=0.766^{+0.02}_{-0.014}\)  [10]}.

The Gaussian prior on \(M_B=-19.244 \pm 0.037\) mag [11]} , corresponding to the SN measurements from \(\rm {SH0ES}\) .

